Radio emission of the nuclei of barred galaxies

Details Radio emission of the nuclei of barred galaxies Radio emission of the nuclei of barred galaxies

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986afz....24...47k&link_type=abstract

(Astrofizika, vol. 24, Jan.-Feb. 1986, p. 47-55) Astrophysics (ISSN 0571-7132), vol. 24, no. 1, July 1986, p. 29-34. Translation

Astronomy and Astrophysics

Astrophysics

8

Barred Galaxies, Emission Spectra, Galactic Nuclei, Radio Spectra, Astronomical Spectroscopy, Spatial Distribution

Scientific paper

It has been shown that the high percentage of radio emission in galaxies of Byurakan classes 2, 2s, 4 and 5 in comparison with classes 1 and 3 is reliably observed only in barred spirals due to galaxies with both central and disk radio components. The radio emission of barred spirals more often than in other types of spirals is connected with the central regions of those galaxies.

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